1203.4000 (Yu. V. Pavlov)
Yu. V. Pavlov
It is shown for the spherically symmetric black holes of the general type that it is impossible to see the infinite future of the Universe external to the hole in the finite proper time interval of the free fall. Quantitative evaluations of the effect of time dilatation for circular orbits around the Kerr black hole are obtained and it is shown that the effect is large for ultrarelativistic energies of the rotating particle.
View original:
http://arxiv.org/abs/1203.4000
No comments:
Post a Comment